Titlebook: Red Dwarfs; Their Geological, Ch David S. Stevenson Book 2019Latest edition Springer Nature Switzerland AG 2019 Habitable worlds.exoplaneta

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FUSE

Conscientious

Exoplanetary Discovery, of 3605 planets had been confirmed, of which 1414 were Neptune-like; by the time this book goes to press that figure will, most likely, be out of date. Therefore, consider this chapter as an incomplete portrait that has many of its key features presented but not all of the hues and textures indicat

護(hù)身符

Deep Cycles and Super-Terrans,n dioxide into the interior in the form of carbonate rock and returns this gas to the atmosphere, thereby modulating the planetary greenhouse effect. One of the more subtle and poorly understood processes is the modulation of surface water—and with it the abundance of many of the ions (both metal an

易彎曲

Atmospheric Circulation and Climate,oing into understanding how planetary atmospheres may influence the same property. This chapter expands upon, improves the accuracy of, and produces viable models of atmospheres for planets with different orbital distances from red dwarf stars.

Vertebra

ETHER

The Niche, Its Hypervolume and the Entropy of Existence,n a few certainties, such as an energy and nutrient source, will life inevitably follow a path to complexity? Although Chaps. 8 and 9 deal with some specifics, this chapter will focus on developing some underlying ideas and principles that are likely to be applicable to all biological systems, no ma

FUSE

The Failure of Early Optimism,, Gliese 581 and Gliese 667C. Both systems hosted a number of super-terrans, whose numbers varied often by the month as radial velocity data was interpreted, reinterpreted, discarded, recovered—only for vexing to continue. Obviously, like many of the authors of the papers upon which the book was cen

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A New Hope, mass red dwarf and the closest star to our Sun, making it a particularly attractive target for further investigation. Meanwhile, the older TRAPPIST-1 system has seven planets, several of which could be habitable—at least in the crudest sense. Although each system has its detractors and flaws, both

ectropion

Book 2019Latest editionhese distant worlds? Could life evolve and survive there? How do these planetary surfaces and geologies evolve? How would life on a planet orbiting a red dwarf differ from life on Earth? And what are the implications for finding further habitable worlds in our galaxy?.The author?provides readers wit